活动星系核的结构与能源机制  

The Structure and Engines of AGNs

作　　者：卢炬甫[1] 

机构地区：[1]中国科学技术大学天体物理中心

出　　处：《天文学进展》1991年第4期271-278,共8页Progress In Astronomy

摘　　要：本文分三部分。首先列举活动星系核的各项基本观测特征;其次是关于这类活动天体的结构,着重讨论宽线区和窄线区的物理性质以及光致电离过程,然后评述能源机制的主流模型即黑洞吸积盘模型,包括星系活动的起因和维持等问题上的最新进展。This article consists of three parts. In the first, basic observational facts of AGNs are listed. The second is devoted to the structure of these objects, with emphasis on the physical properties of the broad line region and the narrow line region, and the process of photoionization. In the last part, the standard model of AGN engines i. e., the black hole accretion disk model, is reviewed, including the most recent progress on the origin and fueling of the galactic activity.

关 键 词：活动星系核 结构 能源机制 

分 类 号：P152[天文地球—天文学]